Spectrograms of the variable star 48 Librae, taken near the last expected minimum, have been examined for irregularities of the shell line profiles. The...
On the simultaneous optical and near-infrared variability of pre-main sequence stars
For a complete understanding of the physical processes causing the photometric variability of pre-main sequence systems, simultaneous optical and near-IR...
On the Sr I λ4607 Å Hanle depolarization signals in the quiet Sun
The Hanle depolarization signals of Sr i λ4607 Å have been used to estimate the unsigned magnetic flux and magnetic energy existing in the quiet Sun photosphere...
On the theory of MAG waves and a comparison with sunspot observations from CDS/SoHO
We examine the influence of non-adiabatic effects on the modes of an isothermal stratified magnetic atmosphere. We present new solutions for magneto-acoustic...
On the use of field RR Lyrae as Galactic probes: VII. Light curve templates in the LSST photometric system
Context. The Vera C. Rubin Observatory will start operations in 2025. During its first two years, too few visits per target per band will be available, meaning...
On the use of photometric redshifts for X-ray selected AGNs
In this paper we present photometric redshift estimates for a sample of X-ray selected sources detected in the wide-field ( 2 deg^2), bright [ f_X(0.5{-}8 keV)...
On the use of the Fourier transform to determine the projected rotational velocity of line-profile variable B stars
Context. The Fourier transform method is a popular tool for deriving the rotational velocities of stars from their spectral line profiles. However, its domain...
On the validity of the 630 nm Fe I lines for magnetometry of the internetwork quiet Sun
Aims.The purpose of this work is to analyze the reliability of the magnetic field strengths inferred from the 630 nm pair of Fe i lines in internetwork quiet...
On the variable spectrum of HD 45677 (FS Canis Majoris)
{ We have studied high-resolution optical spectra of the peculiar B[e] star HD 45677 (FS CMa) observed during 3 nights in October 1995. The main results of our...